Novae (singular nova, Latin for new) are exploding stars.
A "nova" is technically a fusion explosion on the surface of a white dwarf star.
A "supernova" is the end of the cycle of fusion in large stars. The resulting loss of pressure within the star allows the outer layers to collapse, and they are then thrown outward with incredible force.
(for details, see the related questions and link)
A variable star. See related question for more information
Williamina Fleming discovered more than 10,000 stars, in which she discovered 59 gaseous nebulae, 310 variable stars and 10 novae.
No, a nova is a star showing a sudden large increase in brightness and then slowly returning to its original state over a few months. Novae are caused by a cataclysmic nuclear explosion on a white dwarf, which causes a sudden brightening of the star and they can repeat on the same star as material repeatedly builds up on its surface from a nearby companion. They are therefore always in a binary system. Novas/Novea should not be confused with "Supernovae" which are different and are classified into different types.
The elements do not die. The stars collapse into dense dwarf or neutron stars. But many explode as novae and the elements are scattered into space. This is the dust from which the next generation of planets are born.
A nova (as distinct from a supernova) is produced in a close binary system where one member is a white dwarf and the other a larger, less dense star. The white dwarf 'sucks' gas from the larger star which condenses into an accretion disc around the white star's equator. When this accretion disc reaches a critical mass it interacts with material on the white star and produces a huge thermonuclear explosion. This is what we see as a nova event. Novae are variable stars.
Novae Group was created in 2006.
Donatia novae-zelandiae was created in 1853.
Armillaria novae-zelandiae was created in 2001.
Laurelia novae-zelandiae was created in 1838.
Novae Hollandiae Plantarum Specimen was created in 1804.
"Novae" means "new" in Italian.
Supplementum primum Prodromi florae Novae Hollandiae was created in 1830.
Planets cannot become novae; a "nova", or more completely "nova stellarum", is the term given to a "new star" that appears when an old star explodes.
Prodromus Florae Novae Hollandiae et Insulae Van Diemen was created in 1810.
The Latin word nova, meaning new is applied to stars which explode due to any of several instabilities. The plural can be the Latin plural "novae" or English plural "novas".
Slow down 9JFR
The cast of Novae de infinito laudes - 1972 includes: Werner Krenn as Tenor Ingrid Mayr as Alt Edda Moser as Sopran